基于线阵CCD的航空相机镜头焦面的自动定位系统

介绍了一种基于单片机的利用步进电机控制线阵CCD固态传感器来自动准确对镜头焦面定位的一种新方法 ,系统从根本上克服了人为因素在焦距测量中的影响 ,实现了焦距的自动测量 ,具有一定的实用价值。     

大量规则图形傅里叶频谱信息提取方法的研究

在检测系统中,有效的被测信息提取方法是保证检测具有高精度和高效率的主要因素之一。本文提出了大量规则图形傅里叶频谱信息的有效提取方法——频谱点能量包络处理方法,为实现大量规则图形尺寸的高精度和高效率的检测奠定了理论基础。文中还就该方法的应用领域进行了展望。     

航空CCD侦察相机系统研究

根据世界航空CCD相的发展概况，讨论了航空CCD侦察相机系统的技术指标、采用的技术方案和系统实现的技术途径。     

大尺寸弧长图像测量系统及其图像处理方法的研究

基于CCD图像测量技术,提出一种新的非接触大尺寸弧长图像测量系统,该系统可用于测量封闭或非封闭、规则或不规则轮廓的大尺寸弧长。文中给出了系统的结构及原理,并着重讨论了该系统的图像处理方法。最后,利用新系统进行了现场比对实验。     

高分辨率CCD模拟前端系统设计

论述了CCD传感器模拟前端系统设计的关键技术,设计并实现了一种基于高分辨率CCD的模拟前端系统。系统由高分辨率固态成像CCD传感器和高集成度模拟前端处理器件构成,图像数据通过LVDS传输技术发送到后端进行处理。试验测试表明,系统可输出高分辨率图像。     

三维激光扫描测量技术

介绍了三维激光扫描测量系统的技术构成、测量原理,并简要地介绍了法国MENSI三维激光测量系统的技术特点;三维激光扫描测量技术在航空、航天工程中所具有的极其重要的应用价值。     

长焦距TDICCD遥感器光学系统的特点和发展趋势

文章介绍了国外有关长焦距TDI CCD遥感器的研究情况,结合实际的设计经验,系统地阐述了此类系统的特点和其可选的光学系统结构型式的特点,总结出长焦距TDI CCD遥感器光学系统的发展趋势。     

基于多普勒效应的激光微位移测量系统

介绍了一种可进行动态微位移测量的激光微位移测量系统。该系统以多普勒效应为理论基础，以He-Ne激光器为光源，配置了判向变频系统、CCD视频信号的高速动态采集系统、微机处理系统及干涉图像处理软件包等，较传统测量方法其精度、误差、灵敏度及稳定度都有较大提高，并实现了微位移的全自动测量。     

关于CCD相机成像性能评价的扎记

给出了一般情况下面阵CCD元件采样信号强度和相机成像调制传递函数的计算公式,并讨论了线阵CCD(作为面阵CCD的特例)相机成像调制传递函数的变化。     

Advanced Technologies Demonstrated by the Miniature Integrated Camera and Spectrometer (MICAS) Aboard Deep Space 1

MICAS is an integrated multi-channel instrument that includes an ultraviolet imaging spectrometer (80–185 nm), two high-resolution visible imagers (10–20 μrad/pixel, 400–900 nm), and a short-wavelength infrared imaging spectrometer (1250–2600 nm). The wavelength ranges were chosen to maximize the science data that could be collected using existing semiconductor technologies and avoiding the need for multi-octave spectrometers. It was flown on DS1 to validate technologies derived from the development of PICS (Planetary Imaging Camera Spectrometer). These technologies provided a novel systems approach enabling the miniaturization and integration of four instruments into one entity, spanning a wavelength range from the UV to IR, and from ambient to cryogenic temperatures with optical performance at a fraction of a wavelength. The specific technologies incorporated were: a built-in fly-by sequence; lightweight and ultra-stable, monolithic silicon-carbide construction, which enabled room-temperature alignment for cryogenic (85–140 K) performance, and provided superb optical performance and immunity to thermal distortion; diffraction-limited, shared optics operating from 80 to 2600 nm; advanced detector technologies for the UV, visible and short-wavelength IR; high-performance thermal radiators coupled directly to the short-wave infrared (SWIR) detector optical bench, providing an instrument with a mass less than 10 kg, instrument power less than 10 W, and total instrument cost of less than ten million dollars. The design allows the wavelength range to be extended by at least an octave at the short wavelength end and to ∼50 microns at the long wavelength end. Testing of the completed instrument demonstrated excellent optical performance down to 77 K, which would enable a greatly reduced background for longer wavelength detectors. During the Deep Space 1 Mission, MICAS successfully collected images and spectra for asteroid 9969 Braille, Mars, and comet 19/P Borrelly. The Borrelly encounter was a scientific hallmark providing the first clear, high resolution images and excellent, short-wavelength infrared spectra of the surface of an active comet’s nucleus.